1. Special Relativity Einstein messes with space and time

2. 2 How Fast Are You Moving Right Now? 0 m/s relative to your chair0 m/s relative to your chair 400 m/s relative to earth center (rotation)400 m/s relative to earth center (rotation) 30,000 m/s relative to the sun (orbit)30,000 m/s relative to the sun (orbit) 220,000 m/s relative to the galaxy center (orbit)220,000 m/s relative to the galaxy center (orbit) Relative to What?? This is the gist of special relativityThis is the gist of special relativity –it’s the exploration of the physics of relative motion –only relative velocities matter: no absolute frame –very relevant comparative velocity is c = 300,000,000 m/s

3. 3 A world without ether For most of the 19th century, physicists thought that space was permeated by “luminiferous ether”For most of the 19th century, physicists thought that space was permeated by “luminiferous ether” –this was thought to be necessary for light to propagate Michelson and Morley performed an experiment to measure earth’s velocity through this substanceMichelson and Morley performed an experiment to measure earth’s velocity through this substance –first result in 1887 –Michelson was first American to win Nobel Prize in physics Found that light waves don’t bunch up in direction of earth motionFound that light waves don’t bunch up in direction of earth motion –shocked the physics world: no ether!! –speed of light is not measured relative to fixed medium –unlike sound waves, water waves, etc.

4. 4 Einstein’s Two Postulates of Special Relativity The Speed of Light is Constant for any observer, regardless of the motion of the observer or the motion of the light source.The Speed of Light is Constant for any observer, regardless of the motion of the observer or the motion of the light source. The laws of physics are always the same in all inertial ( non-accelerating) frames of reference.The laws of physics are always the same in all inertial ( non-accelerating) frames of reference.

5. 5 Simultaneity is relative, not absolute Observer riding in spaceship at constant velocity sees a flash of light situated in the center of the ship’s chamber hit both ends at the same time But to a stationary observer (or any observer in relative motion), the condition that light travels each way at the same speed in their own frame means that the events will not be simultaneous. In the case pictured, the stationary observer sees the flash hit the back of the ship before the front

6. 6 One person’s space is another’s time If simultaneity is broken, no one can agree on a universal time that suits allIf simultaneity is broken, no one can agree on a universal time that suits all –the relative state of motion is important Because the speed of light is constant (and finite) for all observers, space and time are unavoidably mixedBecause the speed of light is constant (and finite) for all observers, space and time are unavoidably mixed –we’ve seen an aspect of this in that looking into the distance is the same as looking back in time Space and time mixing promotes unified view of spacetimeSpace and time mixing promotes unified view of spacetime –“events” are described by three spatial coordinates plus a time

7. 7 The Lorentz Transformation These Equations Relate the Time and Positions of two Different Frames of ReferenceThese Equations Relate the Time and Positions of two Different Frames of Reference

8. 8 The gamma factor Gamma (  ) is a measure of how relativistic you are:Gamma (  ) is a measure of how relativistic you are: When v = 0,  = 1.0When v = 0,  = 1.0 –and things are normal At v = 0.6c,  = 1.25At v = 0.6c,  = 1.25 –a little strange At v = 0.8c,  = 1.67At v = 0.8c,  = 1.67 –Very strange As v  c, As v  c, 

9. 9 What does  do? Time dilation: clocks on a moving platform appear to tick slower by the factor Time dilation: clocks on a moving platform appear to tick slower by the factor  –standing on platform, you see the clocks on a fast-moving train tick slowly: people age more slowly, though to them, all is normal Length contraction: moving objects appear to be “compressed” along the direction of travel by the factor Length contraction: moving objects appear to be “compressed” along the direction of travel by the factor  –standing on a platform, you see a shorter train slip past, though the occupants see their train as normal length

10. Time Dilation T=  T 0 T=  T 0 T 0 = proper time. It’s measured by the observer who is at rest with respect to the clock T 0 = proper time. It’s measured by the observer who is at rest with respect to the clock T = time measured by the observer that sees the clock moving sees the clock moving Note: only look at one clock in each problem. 10

11. Time Dilation Example A rocket ship moves by you at.866c. The astronaut measures his heart rate at 1beat / second. What do you measure his heart rate to be? T o = 1.00s  = 1/ (1-.866 2 ) 1/2 = 2.00 T o = 1.00s  = 1/ (1-.866 2 ) 1/2 = 2.00 T =  T 0 = 2.00s T =  T 0 = 2.00s One beat every 2 seconds – he’ll live twice as long as you, all things being equal…. One beat every 2 seconds – he’ll live twice as long as you, all things being equal…. 11

12. Time Dilation Example A muon has a lifetime 2 microseconds when it is at rest. What does an observer measure the lifetime to be, when the muons are moving at 99%c? T o = 2  s  = 1/ (1-.99 2 ) 1/2 = 7.10 T o = 2  s  = 1/ (1-.99 2 ) 1/2 = 7.10 T =  T 0 = 14.2  s T =  T 0 = 14.2  s This has been confirmed experimentally. Muons produced in the upper atmosphere should not get to the Earth’s surface – but they do. This has been confirmed experimentally. Muons produced in the upper atmosphere should not get to the Earth’s surface – but they do. 12

13. Length Contraction L= L 0 /  L= L 0 /  L 0 = (proper length) measured by an L 0 = (proper length) measured by an observer that is at rest wrt to the object observer that is at rest wrt to the object L = length measured by an observer watching L = length measured by an observer watching the object move the object move 13

14. Length Contraction Example An astronaut builds a ship 20m long. He passes by you moving at.866c. How long do you say the ship is? L 0 = 20m  = 1/ (1-.866 2 ) 1/2 = 2.00 L 0 = 20m  = 1/ (1-.866 2 ) 1/2 = 2.00 L = 20/(2.00) = 10.0m L = 20/(2.00) = 10.0m 14

15. 15 Why don’t we see relativity every day? We’re soooo slow (relative to c), that length contraction and time dilation don’t amount to muchWe’re soooo slow (relative to c), that length contraction and time dilation don’t amount to much –30 m/s freeway speed has v/c = 10 -7  = 1.000000000000005 –30,000 m/s earth around sun has v/c = 10 -4  = 1.000000005 but precise measurements see this clearly

16. 16 Velocity Addition Also falling out of the requirement that the speed of light is constant for all observers is a new rule for adding velocitiesAlso falling out of the requirement that the speed of light is constant for all observers is a new rule for adding velocities Galilean addition had that someone traveling at v 1 throwing a ball forward at v 2 would make the ball go at v 1 +v 2Galilean addition had that someone traveling at v 1 throwing a ball forward at v 2 would make the ball go at v 1 +v 2 In relativity,In relativity, –reduces to Galilean addition for small velocities –can never get more than c if v 1 and v 2 are both  c –if either v 1 OR v 2 is c, then v rel = c: light always goes at c

17. Velocity Addition Example 17 A spaceship moving at.5c, fires a projectile at.6c in the direction it’s moving. What is the speed of the projectile measured by an observer at rest with respect to the ship? V 1 =.5c V 2 =.6c V rel = (.5c +.6c) / ( 1 + (.5c)(.6c)/c 2 ) = 1.1c / ( 1 +.3) = (1.1)c/(1.3) =.85c NOT 1.1 c ! No correct calculation will ever give you any speed greater than c.

18. Velocity Addition Example A spaceship moving at.5c, fires a laser in the direction it’s moving. What is the speed of the laser light measured by an observer at rest with respect to the ship? V 1 =.5c V 2 = c V 1 =.5c V 2 = c V rel = (.5c + c) / ( 1 + (.5c)(c)/c 2 ) =.6c /.6 V rel = (.5c + c) / ( 1 + (.5c)(c)/c 2 ) =.6c /.6 = c ( it had to be c - the speed of light is = c ( it had to be c - the speed of light is invariant. ) invariant. ) 18

19. 19 Classic Paradoxes The twin paradox:The twin paradox: –one twin (age 30) sets off in rocket at high speed, returns to earth after long trip –if v = 0.6c, 30 years will pass on earth while only 24 will pass in high speed rocket –twin returns at age 54 to find sibling at 60 years old –why not the other way around? –The moving twin is NOT in an inertial system – there is no paradox.

20. 20 What would I experience at light speed? It is impossible to get a massive thing to travel truly at the speed of lightIt is impossible to get a massive thing to travel truly at the speed of light –energy required is  mc 2, where  as v  c –so requires infinite energy to get all the way to c But if you are a massless photon…But if you are a massless photon… –to the outside, your clock is stopped –so you arrive at your destination in the same instant you leave your source (by your clock) across the universe in a perceived instant –makes sense, if to you the outside world’s clock has stopped: you see no “ticks” happen before you hit

21. 21 E total =  mc 2 = mc 2 + 1/2mv 2 Total Energy = Rest energy + Kinetic energy Example: what is the rest energy of a 1kg rock? mc 2 = 1(300,000,000) 2 =90,000,000,000,000,000 Joules

22. 22 Experimental Confirmation We see time dilation in particle lifetimesWe see time dilation in particle lifetimes –in accelerators, particles live longer at high speed their clocks are running slowly as seen by us seen daily in particle accelerators worldwide –cosmic rays make muons in the upper atmosphere these muons only live for about 2 microseconds if not experiencing time dilation, they would decay before reaching the ground, but they do reach the ground in abundance We see length contraction of the lunar orbitWe see length contraction of the lunar orbit –squished a bit in the direction of the earth’s travel around the sun E = mc 2 extensively confirmedE = mc 2 extensively confirmed –nuclear power/bombs –sun’s energy conversion mechanism